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Article: A search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base

TitleA search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base
Authors
Kiss, László L.Moór, AttilaSzalai, TamásKovács, JózsefBayliss, Daniel D RGilmore, Gerard F.Bienaymé, OlivierBinney, James J.Bland-Hawthorn, Joss BlandCampbell, Randy D.Freeman, Kenneth C.Fulbright, Jon P.Gibson, Brad K.Grebel, Eva K.Helmi, AminaMunari, UlisseNavarro, Julio F.Parker, Quentin A.Reid, Warren A.Seabroke, George M.Siebert, ArnaudSiviero, AlessandroSteinmetz, MatthiasWatson, Fred G.Williams, Mary E KWyse, Rosemary F GZwitter, Tomaž
KeywordsOpen clusters and associations: individual: Tucana-Horologium association
Stars: kinematics and dynamics
Open clusters and associations: individual: εCha association
Open clusters and associations: individual: β Pictoris moving group
Issue Date2011
Citation
Monthly Notices of the Royal Astronomical Society, 2011, v. 411, n. 1, p. 117-123 How to Cite?
DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.17660.x
AbstractWe report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow-up high-resolution optical spectroscopy. The results include the identification of one new and five likely members of the βPictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the εCha group and two stars in the Tucana-Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood. © 2010 The Authors. Journal compilation © 2010 RAS.
Persistent Identifierhttp://hdl.handle.net/10722/208919
ISSN
0035-8711
2022 Impact Factor: 4.8
2020 SCImago Journal Rankings: 2.058
ISI Accession Number ID
WOS:000286525600024

 

DC FieldValueLanguage
dc.contributor.authorKiss, László L.-
dc.contributor.authorMoór, Attila-
dc.contributor.authorSzalai, Tamás-
dc.contributor.authorKovács, József-
dc.contributor.authorBayliss, Daniel D R-
dc.contributor.authorGilmore, Gerard F.-
dc.contributor.authorBienaymé, Olivier-
dc.contributor.authorBinney, James J.-
dc.contributor.authorBland-Hawthorn, Joss Bland-
dc.contributor.authorCampbell, Randy D.-
dc.contributor.authorFreeman, Kenneth C.-
dc.contributor.authorFulbright, Jon P.-
dc.contributor.authorGibson, Brad K.-
dc.contributor.authorGrebel, Eva K.-
dc.contributor.authorHelmi, Amina-
dc.contributor.authorMunari, Ulisse-
dc.contributor.authorNavarro, Julio F.-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorReid, Warren A.-
dc.contributor.authorSeabroke, George M.-
dc.contributor.authorSiebert, Arnaud-
dc.contributor.authorSiviero, Alessandro-
dc.contributor.authorSteinmetz, Matthias-
dc.contributor.authorWatson, Fred G.-
dc.contributor.authorWilliams, Mary E K-
dc.contributor.authorWyse, Rosemary F G-
dc.contributor.authorZwitter, Tomaž-
dc.date.accessioned2015-03-23T02:02:11Z-
dc.date.available2015-03-23T02:02:11Z-
dc.date.issued2011-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2011, v. 411, n. 1, p. 117-123-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/208919-
dc.description.abstractWe report on the discovery of new members of nearby young moving groups, exploiting the full power of combining the Radial Velocity Experiment (RAVE) survey with several stellar age diagnostic methods and follow-up high-resolution optical spectroscopy. The results include the identification of one new and five likely members of the βPictoris moving group, ranging from spectral types F9 to M4 with the majority being M dwarfs, one K7 likely member of the εCha group and two stars in the Tucana-Horologium association. Based on the positive identifications, we foreshadow a great potential of the RAVE data base in progressing towards a full census of young moving groups in the solar neighbourhood. © 2010 The Authors. Journal compilation © 2010 RAS.-
dc.languageeng-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectOpen clusters and associations: individual: Tucana-Horologium association-
dc.subjectStars: kinematics and dynamics-
dc.subjectOpen clusters and associations: individual: εCha association-
dc.subjectOpen clusters and associations: individual: β Pictoris moving group-
dc.titleA search for new members of the βPictoris, Tucana-Horologium and εCha moving groups in the RAVE data base-
dc.typeArticle-
dc.description.naturelink_to_OA_fulltext-
dc.identifier.doi10.1111/j.1365-2966.2010.17660.x-
dc.identifier.scopuseid_2-s2.0-78751689898-
dc.identifier.volume411-
dc.identifier.issue1-
dc.identifier.spage117-
dc.identifier.epage123-
dc.identifier.eissn1365-2966-
dc.identifier.isiWOS:000286525600024-
dc.identifier.issnl0035-8711-

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